activity
20192026
most citedA peculiar hard X-ray counterpart of a Galactic fast radio burst

217 citations · 1.2k across the 26 of their papers we have counts for

collaborators
Showing 2024Show all

6 papers · 1 filter

astro-ph.HE2024

Investigating Polarization characteristics of GRB200503A and GRB201009A

Divita Saraogi, Suman Bala, Jitendra Joshi +18

We present results of a comprehensive analysis of the polarization characteristics of GRB 200503A and GRB 201009A observed with the Cadmium Zinc Telluride Imager (CZTI) on board As…

astro-ph.HE2024

The Third Konus-Wind Catalog of Short Gamma-Ray bursts

Alexandra L. Lysenko, Dmitry S. Svinkin, Dmitry D. Frederiks +3

In this catalog, we present the results of a systematic study of 199 short gamma-ray bursts (GRBs) detected by Konus-Wind between 2011 January 1 and 2021 August 31. The catalog ext…

astro-ph.HE2024★ 30 cited

A fast X-ray transient from a weak relativistic jet associated with a type Ic-BL supernova

H. Sun, W. -X. Li, L. -D. Liu +163

Massive stars end their lives as core-collapse supernovae, amongst which some extremes are broad-lined type Ic supernovae from Wolf-Rayet stars associated with long-duration gamma-…

astro-ph.HE2024★ 6 cited

New results on the gamma-ray burst variability-luminosity relation

C. Guidorzi, R. Maccary, A. Tsvetkova +13

At the dawn of the gamma-ray burst (GRB) afterglow era, a Cepheid-like correlation was discovered between time variability V and isotropic-equivalent peak luminosity Liso of the pr…

astro-ph.HE2024★ 2 cited

Soft X-ray prompt emission from a high-redshift gamma-ray burst EP240315a

Y. Liu, H. Sun, D. Xu +191

Long gamma-ray bursts (GRBs) are believed to originate from core collapse of massive stars. High-redshift GRBs can probe the star formation and reionization history of the early un…

astro-ph.HE2024★ 3 cited

The Luminous, Slow-Rising Orphan Afterglow AT2019pim as a Candidate Moderately Relativistic Outflow

Daniel A. Perley, Anna Y. Q. Ho, Michael Fausnaugh +34

Classical gamma-ray bursts (GRBs) have two distinct emission episodes: prompt emission from ultrarelativistic ejecta and afterglow from shocked circumstellar material. While both c…